activity
20082023
most citedA Global Three Dimensional Radiation Magneto-hydrodynamic Simulation of Super-Eddington Accretion Disks

440 citations · 2.5k across the 38 of their papers we have counts for

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Showing 2021Show all

6 papers · 1 filter

astro-ph.GA2021★ 162 cited

A characteristic optical variability timescale in astrophysical accretion disks

Colin J. Burke, Yue Shen, Omer Blaes +8

Accretion disks around supermassive black holes in active galactic nuclei produce continuum radiation at ultraviolet and optical wavelengths. Physical processes in the accretion fl…

astro-ph.GA2021★ 17 cited

The Cosmic Ray Staircase: the Outcome of the Cosmic Ray Acoustic Instability

Tsun Hin Navin Tsung, S. Peng Oh, Yan-Fei Jiang

Recently, cosmic rays (CRs) have emerged as a leading candidate for driving galactic winds. Small-scale processes can dramatically affect global wind properties. We run two-moment…

astro-ph.IM2021

Inferring Black Hole Properties from Astronomical Multivariate Time Series with Bayesian Attentive Neural Processes

Ji Won Park, Ashley Villar, Yin Li +5

Among the most extreme objects in the Universe, active galactic nuclei (AGN) are luminous centers of galaxies where a black hole feeds on surrounding matter. The variability patter…

astro-ph.GA2021★ 45 cited

The Physics of Galactic Winds Driven by Cosmic Rays II: Isothermal Streaming Solutions

Eliot Quataert, Yan-Fei Jiang, Todd A. Thompson

We use analytic calculations and time-dependent spherically-symmetric simulations to study the properties of isothermal galactic winds driven by cosmic-rays (CRs) streaming at the…

astro-ph.EP2021★ 29 cited

Global 3D Radiation Hydrodynamic Simulations of Proto-Jupiter's Convective Envelope

Zhaohuan Zhu, Yan-Fei Jiang, Hans Baehr +3

The core accretion model of giant planet formation has been challenged by the discovery of recycling flows between the planetary envelope and the disc that can slow or stall envelo…

astro-ph.GA2021★ 46 cited

The Physics of Galactic Winds Driven by Cosmic Rays I: Diffusion

Eliot Quataert, Todd A. Thompson, Yan-Fei Jiang

The physics of Cosmic ray (CR) transport remains a key uncertainty in assessing whether CRs can produce galaxy-scale outflows consistent with observations. In this paper, we elucid…